Pith Number
pith:T4LJROTZ
pith:2017:T4LJROTZ4B23IT7L6CHXDIMTJ3
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refs pending
Using the CIFIST grid of CO5BOLD 3D model atmospheres to study the effects of stellar granulation on photometric colours. I. Grids of 3D corrections in the UBVRI, 2MASS, Hipparcos, Gaia, and SDSS systems
arxiv:1712.00024 v2 · 2017-11-30 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{T4LJROTZ4B23IT7L6CHXDIMTJ3}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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4
Citations
5
Replications
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Portable graph bundle live · download bundle · merged
state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Receipt and verification
| First computed | 2026-05-18T00:19:24.847519Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9f1698ba79e075b44febf08f71a1934ef234134af9e8663f75e69b926c25c8c9
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/T4LJROTZ4B23IT7L6CHXDIMTJ3 \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 9f1698ba79e075b44febf08f71a1934ef234134af9e8663f75e69b926c25c8c9
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7535a05f28befa3400c87ced73d12ca84d210ef60156adc4910de60a4ef0f9dc",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2017-11-30T19:00:06Z",
"title_canon_sha256": "0f84246c1a01f572c7da91863fab383a064593b61b068ad87162d43b98ee2870"
},
"schema_version": "1.0",
"source": {
"id": "1712.00024",
"kind": "arxiv",
"version": 2
}
}